H-ATLAS/GAMA: Quantifying the morphological evolution of the galaxy population using cosmic calorimetry

Stephen Eales; Andrew Fullard; Matthew Allen; M. W. L. Smith; Ivan Baldry; Nathan Bourne; C. J. R. Clark; Simon Driver; Loretta Dunne; Simon Dye; Alister W. Graham; Edo Ibar; Andrew Hopkins; Rob Ivison; Lee S. Kelvin; Steve Maddox; Claudia Maraston; Aaron S. G. Robotham; Daniel Smith; Edward N. Taylor; Elisabetta Valiante; Paul van der Werf; Maarten Baes; Sarah Brough; David Clements; Asantha Cooray; Haley Gomez; Jon Loveday; Steven Phillipps; Douglas Scott; Steve Serjeant

doi:10.1093/mnras/stv1300

H-ATLAS/GAMA: Quantifying the morphological evolution of the galaxy population using cosmic calorimetry

Stephen Eales
, Andrew Fullard
, Matthew Allen
, M. W. L. Smith
, Ivan Baldry
, Nathan Bourne
, C. J. R. Clark
, Simon Driver
, Loretta Dunne
, Simon Dye
, Alister W. Graham
, Edo Ibar
, Andrew Hopkins
, Rob Ivison
, Lee S. Kelvin
, Steve Maddox
, Claudia Maraston
, Aaron S. G. Robotham
, Daniel Smith
, Edward N. Taylor

Elisabetta Valiante, Paul van der Werf, Maarten Baes, Sarah Brough, David Clements, Asantha Cooray, Haley Gomez, Jon Loveday, Steven Phillipps, Douglas Scott, Steve Serjeant

Research output: Contribution to journal › Article › peer-review

18 Citations (Scopus)

113 Downloads (Pure)

Abstract

Using results from the Herschel Astrophysical Terrahertz Large-Area Survey and the Galaxy and Mass Assembly project, we show that, for galaxy masses above approximately 1.0e8 solar masses, 51% of the stellar mass-density in the local Universe is in early-type galaxies (ETGs: Sersic n > 2.5) while 89% of the rate of production of stellar mass-density is occurring in late-type galaxies (LTGs: Sersic n

Original language	English
Pages (from-to)	3489-3507
Journal	Monthly Notices of the Royal Astronomical Society (MNRAS)
Volume	452
Issue number	4
Early online date	20 Aug 2015
DOIs	https://doi.org/10.1093/mnras/stv1300
Publication status	Published - 1 Oct 2015

Keywords

astro-ph.GA
astro-ph.CO

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10.1093/mnras/stv1300

pdfAccepted author manuscript, 4.4 MB

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Eales, S., Fullard, A., Allen, M., Smith, M. W. L., Baldry, I., Bourne, N., Clark, C. J. R., Driver, S., Dunne, L., Dye, S., Graham, A. W., Ibar, E., Hopkins, A., Ivison, R., Kelvin, L. S., Maddox, S., Maraston, C., Robotham, A. S. G., Smith, D., ... Serjeant, S. (2015). H-ATLAS/GAMA: Quantifying the morphological evolution of the galaxy population using cosmic calorimetry. Monthly Notices of the Royal Astronomical Society (MNRAS), 452(4), 3489-3507. https://doi.org/10.1093/mnras/stv1300

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title = "H-ATLAS/GAMA: Quantifying the morphological evolution of the galaxy population using cosmic calorimetry",

abstract = "Using results from the Herschel Astrophysical Terrahertz Large-Area Survey and the Galaxy and Mass Assembly project, we show that, for galaxy masses above approximately 1.0e8 solar masses, 51\% of the stellar mass-density in the local Universe is in early-type galaxies (ETGs: Sersic n > 2.5) while 89\% of the rate of production of stellar mass-density is occurring in late-type galaxies (LTGs: Sersic n",

keywords = "astro-ph.GA, astro-ph.CO",

author = "Stephen Eales and Andrew Fullard and Matthew Allen and Smith, \{M. W. L.\} and Ivan Baldry and Nathan Bourne and Clark, \{C. J. R.\} and Simon Driver and Loretta Dunne and Simon Dye and Graham, \{Alister W.\} and Edo Ibar and Andrew Hopkins and Rob Ivison and Kelvin, \{Lee S.\} and Steve Maddox and Claudia Maraston and Robotham, \{Aaron S. G.\} and Daniel Smith and Taylor, \{Edward N.\} and Elisabetta Valiante and Werf, \{Paul van der\} and Maarten Baes and Sarah Brough and David Clements and Asantha Cooray and Haley Gomez and Jon Loveday and Steven Phillipps and Douglas Scott and Steve Serjeant",

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doi = "10.1093/mnras/stv1300",

language = "English",

volume = "452",

pages = "3489--3507",

journal = "Monthly Notices of the Royal Astronomical Society (MNRAS)",

issn = "0035-8711",

publisher = "Oxford University Press (OUP)",

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Eales, S, Fullard, A, Allen, M, Smith, MWL, Baldry, I, Bourne, N, Clark, CJR, Driver, S, Dunne, L, Dye, S, Graham, AW, Ibar, E, Hopkins, A, Ivison, R, Kelvin, LS, Maddox, S, Maraston, C, Robotham, ASG, Smith, D, Taylor, EN, Valiante, E, Werf, PVD, Baes, M, Brough, S, Clements, D, Cooray, A, Gomez, H, Loveday, J, Phillipps, S, Scott, D & Serjeant, S 2015, 'H-ATLAS/GAMA: Quantifying the morphological evolution of the galaxy population using cosmic calorimetry', Monthly Notices of the Royal Astronomical Society (MNRAS), vol. 452, no. 4, pp. 3489-3507. https://doi.org/10.1093/mnras/stv1300

TY - JOUR

T1 - H-ATLAS/GAMA

T2 - Quantifying the morphological evolution of the galaxy population using cosmic calorimetry

AU - Eales, Stephen

AU - Fullard, Andrew

AU - Allen, Matthew

AU - Smith, M. W. L.

AU - Baldry, Ivan

AU - Bourne, Nathan

AU - Clark, C. J. R.

AU - Driver, Simon

AU - Dunne, Loretta

AU - Dye, Simon

AU - Graham, Alister W.

AU - Ibar, Edo

AU - Hopkins, Andrew

AU - Ivison, Rob

AU - Kelvin, Lee S.

AU - Maddox, Steve

AU - Maraston, Claudia

AU - Robotham, Aaron S. G.

AU - Smith, Daniel

AU - Taylor, Edward N.

AU - Valiante, Elisabetta

AU - Werf, Paul van der

AU - Baes, Maarten

AU - Brough, Sarah

AU - Clements, David

AU - Cooray, Asantha

AU - Gomez, Haley

AU - Loveday, Jon

AU - Phillipps, Steven

AU - Scott, Douglas

AU - Serjeant, Steve

PY - 2015/10/1

Y1 - 2015/10/1

N2 - Using results from the Herschel Astrophysical Terrahertz Large-Area Survey and the Galaxy and Mass Assembly project, we show that, for galaxy masses above approximately 1.0e8 solar masses, 51% of the stellar mass-density in the local Universe is in early-type galaxies (ETGs: Sersic n > 2.5) while 89% of the rate of production of stellar mass-density is occurring in late-type galaxies (LTGs: Sersic n

AB - Using results from the Herschel Astrophysical Terrahertz Large-Area Survey and the Galaxy and Mass Assembly project, we show that, for galaxy masses above approximately 1.0e8 solar masses, 51% of the stellar mass-density in the local Universe is in early-type galaxies (ETGs: Sersic n > 2.5) while 89% of the rate of production of stellar mass-density is occurring in late-type galaxies (LTGs: Sersic n

KW - astro-ph.GA

KW - astro-ph.CO

U2 - 10.1093/mnras/stv1300

DO - 10.1093/mnras/stv1300

M3 - Article

SN - 0035-8711

VL - 452

SP - 3489

EP - 3507

JO - Monthly Notices of the Royal Astronomical Society (MNRAS)

JF - Monthly Notices of the Royal Astronomical Society (MNRAS)

IS - 4

ER -

H-ATLAS/GAMA: Quantifying the morphological evolution of the galaxy population using cosmic calorimetry

Abstract

Keywords

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